Accepted author manuscript, 5.79 MB, PDF document
Available under license: CC BY: Creative Commons Attribution 4.0 International License
Final published version
Licence: CC BY: Creative Commons Attribution 4.0 International License
Research output: Contribution to Journal/Magazine › Journal article › peer-review
Research output: Contribution to Journal/Magazine › Journal article › peer-review
}
TY - JOUR
T1 - J-PLUS
T2 - Uncovering a large population of extreme [OIII] emitters in the local Universe
AU - Lumbreras-Calle, A.
AU - López-Sanjuan, C.
AU - Sobral, D.
AU - Fernández-Ontiveros, J. A.
AU - Vílchez, J. M.
AU - Hernán-Caballero, A.
AU - Akhlaghi, M.
AU - Díaz-García, L. A.
AU - Alcaniz, J.
AU - Angulo, R. E.
AU - Cenarro, A. J.
AU - Cristóbal-Hornillos, D.
AU - Dupke, R. A.
AU - Ederoclite, A.
AU - Hernández-Monteagudo, C.
AU - Marín-Franch, A.
AU - Moles, M.
AU - Jr, L. Sodré
AU - Ramió, H. Vázquez
AU - Varela, J.
N1 - 22 pages, 22 figures. Submitted to Astronomy & Astrophysics
PY - 2022/12/31
Y1 - 2022/12/31
N2 - Over the past decades, several studies have discovered a population of galaxies undergoing very strong star formation events, called extreme emission line galaxies (EELGs). In this work, we exploit the capabilities of the Javalambre Photometric Local Universe Survey (J-PLUS), a wide field multifilter survey, with 2000 square degrees observed. We use it to identify EELGs at low redshift by their [OIII]5007 emission line. We intend to provide with a more complete, deep, and less biased sample of local EELGs. We select objects with an excess of flux in the J-PLUS mediumband $J0515$ filter, which covers the [OIII] line at z$
AB - Over the past decades, several studies have discovered a population of galaxies undergoing very strong star formation events, called extreme emission line galaxies (EELGs). In this work, we exploit the capabilities of the Javalambre Photometric Local Universe Survey (J-PLUS), a wide field multifilter survey, with 2000 square degrees observed. We use it to identify EELGs at low redshift by their [OIII]5007 emission line. We intend to provide with a more complete, deep, and less biased sample of local EELGs. We select objects with an excess of flux in the J-PLUS mediumband $J0515$ filter, which covers the [OIII] line at z$
KW - astro-ph.GA
U2 - 10.1051/0004-6361/202142898
DO - 10.1051/0004-6361/202142898
M3 - Journal article
VL - 668
JO - Astronomy and Astrophysics
JF - Astronomy and Astrophysics
SN - 1432-0746
M1 - A60
ER -